Microlensing Black Hole
About This Image
Caption
The star-filled sky in this Hubble Space Telescope photo is located in the direction of the Galactic center. The brightness of stars are monitored to see if any change in apparent brightness is made by a foreground object drifting in front of them. The warping of space by the interloper would momentarily brighten the appearance of a background star, due to an effect called gravitational lensing. One such event is shown along the four close-up frames at the bottom. The arrow points to a star that momentarily brightened, as first captured by Hubble beginning in August, 2011. This was caused by a foreground black hole drifting in front of the star, along our line-of-sight. The star brightened and then subsequently faded back to its normal brightness as the black hole passed by. Because a black hole doesn't emit or reflect light, it cannot be directly observed. But its unique thumbprint on the fabric of space can be measured through these so-called microlensing events. Though an estimated 100 million isolated black holes roam our galaxy, finding the telltale signature of one is a needle-in-haystack search for Hubble astronomers.
Credits
SCIENCE:
NASA, ESA, Kailash
Sahu
(STScI)
IMAGE PROCESSING:
Joseph
DePasquale
(STScI)
Keywords
| About The Object | |
|---|---|
| Object Name | OGLE-2011-BLG-462 |
| Object Description | Microlensing black hole |
| R.A. Position | 17:51:41.9 |
| Dec. Position | -29:37:27.2 |
| Constellation | Ophiuchus |
| Distance | 5,000 light-years |
| About The Data | |
| Data Description | The HST observations include those from programs 12322 , 12670 and 14783 (K. Sahu) |
| Instrument | WFC3/UVIS |
| Exposure Dates | 8 Aug. 2011, 31 Oct. 2011, 9 Sept. 2012 and 29 Aug. 2017 |
| Filters | F606W and F814W |
| About The Image | |
| Color Info | These images are a composite of separate exposures acquired by the WFC3 instrument on the Hubble Space Telescope. Several filters were used to sample wide wavelength ranges. The color results from assigning different hues (colors) to each monochromatic (greyscale) image associated with an individual filter. In this case, the assigned colors are:
Cyan: F606W Orange: F814W |
| Compass Image |  |
| About The Object | |
|---|---|
| Object Name | A name or catalog number that astronomers use to identify an astronomical object. |
| Object Description | The type of astronomical object. |
| R.A. Position | Right ascension – analogous to longitude – is one component of an object's position. |
| Dec. Position | Declination – analogous to latitude – is one component of an object's position. |
| Constellation | One of 88 recognized regions of the celestial sphere in which the object appears. |
| Distance | The physical distance from Earth to the astronomical object. Distances within our solar system are usually measured in Astronomical Units (AU). Distances between stars are usually measured in light-years. Interstellar distances can also be measured in parsecs. |
| Dimensions | The physical size of the object or the apparent angle it subtends on the sky. |
| About The Data | |
| Data Description |
|
| Instrument | The science instrument used to produce the data. |
| Exposure Dates | The date(s) that the telescope made its observations and the total exposure time. |
| Filters | The camera filters that were used in the science observations. |
| About The Image | |
| Image Credit | The primary individuals and institutions responsible for the content. |
| Publication Date | The date and time the release content became public. |
| Color Info | A brief description of the methods used to convert telescope data into the color image being presented. |
| Orientation | The rotation of the image on the sky with respect to the north pole of the celestial sphere. |